Shortly after the seminal paper “Self-Organized Criticality: An explanation of 1/f noise” by
Bak et al.(1987), the idea has been applied to solar physics, in “Avalanches and the …

This paper is a pedagogical introduction to avalanche models of solar flares, including a
comprehensive review of recent modeling efforts and directions. This class of flare model is …

A derivation in variable dimension of the scaling laws for mixed third-order longitudinal
structure and correlation functions for incompressible magnetized flows is given for arbitrary …

The heating of the solar corona has been a fundamental astrophysical issue for over sixty
years. Over the last decade in particular, space-based solar observatories (Yohkoh, SOHO …

The following chapter provides an overview of the techniques used to understand Self-
Organised Criticality (SOC) by performing computer simulations. Those are of particular …

We present a statistical survey of almost 10,000 radio type III bursts observed by the Nançay
Radioheliograph from 1998 to 2008, covering nearly a full solar cycle. In particular, sources …

We review the current literature on the formation of coherent structures (CoSs) in strongly
turbulent 3D magnetized plasmas. CoSs [Current Sheets (CS), magnetic filaments, large …

The long-time statistical behavior of a two-dimensional section of a coronal loop subject to
random magnetic forcing is presented. The highly intermittent nature of dissipation is …

Aims. We investigate the statistics for the spatial and temporal distribution of the energy input
into the corona in a three-dimensional magneto-hydrodynamical (3D MHD) model. The …

We report low-frequency (80 MHz) radio observations of circularly polarized non-thermal
type I radio bursts (" noise storms") in the solar corona whose estimated energy is∼ 10 21 …